Subject |
has part mean Ni content of sulfide |
has weather resistance |
has part carbon |
has synonym |
has olivine shock metamorphism |
has part matrix |
is independent of |
has shock pressure |
has degree of aqueous alteration |
has matrix abundance |
has petrologic subtype |
has sediment mechanism |
has image |
has weather |
has degree of secondary process |
has part feldspar |
has metal abundance |
has refractory inclusion abundance |
has relative abundance |
has fragmentation probability |
has chondrule mean diameter |
has metamorphism mechanism |
is a kind of |
has age |
has part sulfide Ni content |
has part maximum bulk Ni in metal |
has total iron content |
has definition |
has number of find |
has petrologic type |
has find date |
has part water |
has degree of thermal metamorphism |
has orthopyroxene shock metamorphism |
has plagioclase shock metamorphism |
has iron metal and iron sulfide |
has degree of shock metamorphism |
has mass |
has abundance |
has peak temperature |
has shock diagnostic mineral |
has name |
be shock |
has fall location |
is an instance of |
has shock stage |
has part metal maximum bulk |
has homogeneity of olivine and low Ca pyroxene |
has structural state of low Ca pyroxene |
has value |
has fall coordinate |
has olivine and low Ca pyroxene homogeneity |
has ablative mass loss |
has total mass of find |
has chondrule abundance |
has parent body |
has part chondrule |
has metal iron content |
has petrologic type range |
H3 chondrite | in weight % | low | 0.2 to 1 % by weight | bronzite chondrite | | clastic and minor opaque | | | none | 10 to 15 % by volume | | agglomeration of particles, many of which record individual, diverse histories | | | | minor primary grains only | 10 % by volume | 0.1 to 1 % by volume | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | 0.3 millimeters | | type 3 chondrite | oldest and most primitive rock in solar system | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | high | | 9 | 3 | | 0.3 to 3 % by weight | none | | | 75 % of total iron | | | most common chondrite observed from falls | less than 950 degree Celsius during its entire history since solidification | | based on the locale, region, or nearby town in which the fall occurred | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | in weight % | definition goes here | predominantly monoclinic | | in degrees, minutes and seconds of lattitude and longitude | greater than 5 % deviations | high because it is more friable than iron meteorite | 349 kg | 60 to 80 % by volume | asteroid smaller than 100 km in diameter | chondrules very sharply defined | 12 to 21 % | which depends on degree of aqueous alteration and thermal metamorphism |
meteorite find | | which depends on its composition | | | | | | | | | | | | can be severe due to long exposure time to environmental corrosion agents | | | | | | during meteor phase which depends on composition | | | meteorite | | | | | a meteorite whose fall was not witnessed | 1691 | | when the meteorite was found | | | | | | | | | | | based on the locale, region, or nearby town in which the fall occurred | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | | | | lower because the fall was not witnessed | in degrees, minutes and seconds of lattitude and longitude | | directly proportional to initial velocity | 485755 kg | | | | | |
S1 shock stage chondrite | in weight % | which depends on its composition | in weight % | | sharp optical extinction, irregular fractures | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | the nature and degree of thermal metamorphism or aqueous alteration | less than 5 GPa | | in volume % | | agglomeration of particles, many of which record individual, diverse histories | | | providing insight into geological evolution of parent asteroid | usually plagioclase tectosilicate | in volume % | in volume % | | during meteor phase which depends on composition | millimeters | shock metamorphism | S1 shock stage meteorite | oldest and most primitive rock in solar system | | | | | 1691 | | | in weight % | | sharp optical extinction, irregular fractures | sharp optical extinction, irregular fractures | | unshocked | | | less than 950 degree Celsius during its entire history since solidification | orthopyroxene for enstatite chondrite | based on the locale, region, or nearby town in which the fall occurred | before, during or after other types of metamorphism | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | S1 | in weight % | definition goes here | definition goes here | | in degrees, minutes and seconds of lattitude and longitude | | directly proportional to initial velocity | 485755 kg | in volume % | asteroid smaller than 100 km in diameter | small sphere of about 1 mm diameter of formerly melted minerals | | which depends on degree of aqueous alteration and thermal metamorphism |
Grady (1937) | in weight % | which depends on its composition | 0.2 to 1 % by weight | bronzite chondrite | sharp optical extinction, irregular fractures | clastic and minor opaque | the nature and degree of thermal metamorphism or aqueous alteration | less than 5 GPa | none | 10 to 15 % by volume | 3.7 | agglomeration of particles, many of which record individual, diverse histories |
 | can be severe due to long exposure time to environmental corrosion agents | providing insight into geological evolution of parent asteroid | minor primary grains only | 10 % by volume | 0.1 to 1 % by volume | | during meteor phase which depends on composition | 0.3 millimeters | shock metamorphism | | oldest and most primitive rock in solar system | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | high | | 9 | 3 | 1937 | 0.3 to 3 % by weight | none | sharp optical extinction, irregular fractures | sharp optical extinction, irregular fractures | 75 % of total iron | unshocked | 9.3 kg | most common chondrite observed from falls | less than 950 degree Celsius during its entire history since solidification | orthopyroxene for enstatite chondrite | Grady (1937) | before, during or after other types of metamorphism | Grady, New Mexico | S1 shock stage chondrite | S1 | in weight % | definition goes here | predominantly monoclinic | lower because the fall was not witnessed | 34° 48' N., 103° 19' W. | greater than 5 % deviations | directly proportional to initial velocity | 349 kg | 60 to 80 % by volume | asteroid smaller than 100 km in diameter | chondrules very sharply defined | 12 to 21 % | which depends on degree of aqueous alteration and thermal metamorphism |